activity
20152025
most citedA large light-mass component of cosmic rays at 10^{17} - 10^{17.5} eV from radio observations

156 citations · 660 across the 13 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020★ 131 cited

Chromatic periodic activity down to 120 MHz in a Fast Radio Burst

Inés Pastor-Marazuela, Liam Connor, Joeri van Leeuwen +34

Fast radio bursts (FRBs) are extragalactic astrophysical transients whose brightness requires emitters that are highly energetic, yet compact enough to produce the short, milliseco…

physics.ao-ph2020★ 25 cited

The initial stage of cloud lightning imaged in high-resolution

O. Scholten, B. M. Hare, J. Dwyer +21

With LOFAR we have been able to image the development of lightning flashes with meter-scale accuracy and unprecedented detail. We discuss the primary steps behind our most recent l…

physics.ao-ph2020★ 46 cited

Radio emission from negative lightning leader steps reveals inner meter-scale structure

B. M. Hare, O. Scholten, J. Dwyer +19

We use the Low Frequency ARray (LOFAR) to probe the dynamics of the stepping process of negatively-charged plasma channels (negative leaders) in a lightning discharge. We observe t…

astro-ph.HE2020★ 26 cited

Reconstructing air shower parameters with LOFAR using event specific GDAS atmospheres

P. Mitra, A. Bonardi, A. Corstanje +15

The limited knowledge of atmospheric parameters like humidity, pressure, temperature, and the index of refraction has been one of the important systematic uncertainties in reconstr…

astro-ph.HE2020★ 13 cited

On the cosmic-ray energy scale of the LOFAR radio telescope

K. Mulrey, S. Buitink, A. Corstanje +14

Cosmic rays are routinely measured at LOFAR, both with a dense array of antennas and with the LOFAR Radboud air shower Array (LORA) which is an array of plastic scintillators. In t…

astro-ph.HE2020★ 66 cited

Repeating fast radio bursts with WSRT/Apertif

L. C. Oostrum, Y. Maan, J. van Leeuwen +40

Repeating fast radio bursts (FRBs) present excellent opportunities to identify FRB progenitors and host environments, as well as decipher the underlying emission mechanism. Detaile…